The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy

Autores
Sandor, Zsolt; Maffione, Nicolás Pablo
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión aceptada
Descripción
Fil: Sandor, Zsolt. Konkoly Observatory of the Hungarian Academy of Sciences; Hungría.
Fil: Maffione, Nicolás P. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Grupo de Caos en Sistemas Hamiltonianos; Argentina
A recently introduced chaos detection method, the Relative Lyapunov Indicator (RLI) is investigated in the cases of symplectic mappings and continuous Hamiltonian systems. It is shown that the RLI is an efficient numerical tool in determining the true nature of individual orbits, and in separating ordered and chaotic regions of the phase space of dynamical systems. A comparison between the RLI and some other variational indicators are presented, as well as the recent applications of the RLI to various problems of dynamical astronomy.
Materia
Planetary System
Giant Planet
Chaotic Orbit
Regular Orbit
Dark Matter Halo
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
RID-UNRN (UNRN)
Institución
Universidad Nacional de Río Negro
OAI Identificador
oai:rid.unrn.edu.ar:20.500.12049/3766

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network_name_str RID-UNRN (UNRN)
spelling The Relative Lyapunov Indicators: Theory and Application to Dynamical AstronomySandor, ZsoltMaffione, Nicolás PabloPlanetary SystemGiant PlanetChaotic OrbitRegular OrbitDark Matter HaloFil: Sandor, Zsolt. Konkoly Observatory of the Hungarian Academy of Sciences; Hungría.Fil: Maffione, Nicolás P. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Grupo de Caos en Sistemas Hamiltonianos; ArgentinaA recently introduced chaos detection method, the Relative Lyapunov Indicator (RLI) is investigated in the cases of symplectic mappings and continuous Hamiltonian systems. It is shown that the RLI is an efficient numerical tool in determining the true nature of individual orbits, and in separating ordered and chaotic regions of the phase space of dynamical systems. A comparison between the RLI and some other variational indicators are presented, as well as the recent applications of the RLI to various problems of dynamical astronomy.Springer2015-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfSándor Z., Maffione N. (2016) The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy. In: Skokos C., Gottwald G., Laskar J. (eds) Chaos Detection and Predictability. Lecture Notes in Physics, vol 915. Springer, Berlin, Heidelberg0075-8450https://rid.unrn.edu.ar/jspui/handle/20.500.12049/3766https://doi.org/10.1007/978-3-662-48410-4_6eng915Lecture Notes in Physicsinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/reponame:RID-UNRN (UNRN)instname:Universidad Nacional de Río Negro2025-10-23T11:17:38Zoai:rid.unrn.edu.ar:20.500.12049/3766instacron:UNRNInstitucionalhttps://rid.unrn.edu.ar/jspui/Universidad públicaNo correspondehttps://rid.unrn.edu.ar/oai/snrdrid@unrn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:43692025-10-23 11:17:38.447RID-UNRN (UNRN) - Universidad Nacional de Río Negrofalse
dc.title.none.fl_str_mv The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
title The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
spellingShingle The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
Sandor, Zsolt
Planetary System
Giant Planet
Chaotic Orbit
Regular Orbit
Dark Matter Halo
title_short The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
title_full The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
title_fullStr The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
title_full_unstemmed The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
title_sort The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
dc.creator.none.fl_str_mv Sandor, Zsolt
Maffione, Nicolás Pablo
author Sandor, Zsolt
author_facet Sandor, Zsolt
Maffione, Nicolás Pablo
author_role author
author2 Maffione, Nicolás Pablo
author2_role author
dc.subject.none.fl_str_mv Planetary System
Giant Planet
Chaotic Orbit
Regular Orbit
Dark Matter Halo
topic Planetary System
Giant Planet
Chaotic Orbit
Regular Orbit
Dark Matter Halo
dc.description.none.fl_txt_mv Fil: Sandor, Zsolt. Konkoly Observatory of the Hungarian Academy of Sciences; Hungría.
Fil: Maffione, Nicolás P. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Grupo de Caos en Sistemas Hamiltonianos; Argentina
A recently introduced chaos detection method, the Relative Lyapunov Indicator (RLI) is investigated in the cases of symplectic mappings and continuous Hamiltonian systems. It is shown that the RLI is an efficient numerical tool in determining the true nature of individual orbits, and in separating ordered and chaotic regions of the phase space of dynamical systems. A comparison between the RLI and some other variational indicators are presented, as well as the recent applications of the RLI to various problems of dynamical astronomy.
description Fil: Sandor, Zsolt. Konkoly Observatory of the Hungarian Academy of Sciences; Hungría.
publishDate 2015
dc.date.none.fl_str_mv 2015-01
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/acceptedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str acceptedVersion
dc.identifier.none.fl_str_mv Sándor Z., Maffione N. (2016) The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy. In: Skokos C., Gottwald G., Laskar J. (eds) Chaos Detection and Predictability. Lecture Notes in Physics, vol 915. Springer, Berlin, Heidelberg
0075-8450
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/3766
https://doi.org/10.1007/978-3-662-48410-4_6
identifier_str_mv Sándor Z., Maffione N. (2016) The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy. In: Skokos C., Gottwald G., Laskar J. (eds) Chaos Detection and Predictability. Lecture Notes in Physics, vol 915. Springer, Berlin, Heidelberg
0075-8450
url https://rid.unrn.edu.ar/jspui/handle/20.500.12049/3766
https://doi.org/10.1007/978-3-662-48410-4_6
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 915
Lecture Notes in Physics
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/4.0/
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv reponame:RID-UNRN (UNRN)
instname:Universidad Nacional de Río Negro
reponame_str RID-UNRN (UNRN)
collection RID-UNRN (UNRN)
instname_str Universidad Nacional de Río Negro
repository.name.fl_str_mv RID-UNRN (UNRN) - Universidad Nacional de Río Negro
repository.mail.fl_str_mv rid@unrn.edu.ar
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